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首页> 外文期刊>Bulletin of the Russian Academy of Sciences. Physics >Antiprotons of Galactic Cosmic Radiation in the PAMELA Experiment
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Antiprotons of Galactic Cosmic Radiation in the PAMELA Experiment

机译:PAMELA实验中银河宇宙辐射的反质子

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摘要

A method for antiproton selection against a background of electrons, based on a mathematical model of data classification using variations in interparticle interaction in a calorimeter, and a method for excluding events accompanied by scattering in the inner detectors of a tracking system (which result in errors in the measured trajectory's curvature and charge sign) from analysis are discussed in this paper.Antiproton spectra and antiproton/proton flux ratio at energies of 0.06 to 350 GeV with statistics of events surpassing those in [1] are obtained.The results can be used to create models for the generation and distribution of particles in the Galaxy, and for searching and studying the nature of hypothetical dark matter particles.
机译:一种基于电子背景的反质子选择方法,该方法基于使用量热计中粒子间相互作用的变化进行数据分类的数学模型,以及一种用于排除跟踪系统内部检测器中伴随散射的事件的方法(这会导致错误)本文讨论了从分析中得到的轨迹的曲率和电荷符号的变化。在能量为0.06至350 GeV的情况下,反质子谱和反质子/质子通量比得到了超过[1]中的事件统计值。创建模型以在银河系中生成和分布粒子,并搜索和研究假设的暗物质粒子的性质。

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